Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
UCB / SSL
U. C. Berkeley
California Univ., Berkeley
Stanford University, Stanford, CA, US
Stanford University, CA
California, University, Berkeley
Stanford Univ., CA.
Space Science Lab UC Berkeley, 7 Gauss Way, Berkeley, CA 94720-7450, USA
Space Sciences Laboratory, University of California, Berkeley, USA
Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450, USA
Space Sciences Laboratory, University of California Berkeley, CA 94720-7450, USA
UC / Berkeley
Space Sciences Lab, University of California
UC-Berkeley
SSL
Los Alamos National Lab., NM.
Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450
University of California, Berkeley
Space Sciences Lab, UC Berkeley
UCB
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA Sciences Laboratory, University of California at Berkeley, 7 Gauss Way, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California, 7 Gauss Way, Berkeley, CA 94720, USA
Space Sciences Lab, U.C. Berkeley, 7 Gauss Way, Berkeley, CA 94597, USA
Space Sciences Laboratory, 7 Gauss Way, University of California, Berkeley, 94720-7450, USA
Space Sciences Lab, University of California, 7 Gauss Way, Berkeley, CA 94720, USA
Space Sciences Lab, University of California, Berkeley, CA, USA
Space Sciences Laboratory, University of California, Berkeley, CA, USA
Space Sciences Laboratory, UC Berkeley, 7 Gauss Way, Berkeley, CA 94720-7450, USA
SSL, UC Berkeley, Space Sciences Lab # 7450 University of California 7 Gauss Way, Berkeley, CA 94720-7450, USA
Space Sciences Laboratory, Univ California Berkeley, Berkeley, CA, USA
"Relationship between flare X-rays and photospheric magnetic fields"
A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953
A Numerical Package for Modeling Solar Flares and Interpreting HESSI Data
A RHESSI search for chromospheric evaporation in super-hot flares
An upper limit of the number and energy of electrons accelerated at an extended coronal shock wave
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